The galaxy presents as a relatively small, disk-shaped structure oriented approximately edge-on to our line of sight. A bright, concentrated central bulge is apparent, exhibiting a slightly elongated morphology. Perpendicular to the central bulge, faint extensions suggestive of spiral arms appear to emanate. These extensions exhibit a mottled appearance with varying luminosity, potentially indicating areas of active star formation or dust obscuration. The color gradient shifts from a bluer hue in the outer regions to a redder hue towards the central bulge, possibly reflecting differences in stellar populations or dust content. There are indications of potential disturbances within the galaxy’s structure, but further observations are needed to determine if this is an ongoing merger event, a tidal interaction, or a result of internal dynamic processes. Overall, the galaxy displays characteristics of a spiral galaxy with moderate disturbances and active regions.
