The galaxy presents as a relatively compact, disk-shaped structure with a noticeable bulge. The disk exhibits a moderately inclined orientation relative to our line of sight. The central region is dominated by yellowish light, suggestive of an older stellar population and potentially a more massive, quiescent core. Moving outward from the center, there is a transition to greenish hues, particularly in the outer disk regions. This color gradient indicates the presence of younger, actively star-forming regions with ionized gas. There is no strong evidence of significant tidal disturbances or ongoing major mergers affecting the galaxy's overall morphology.
