The galaxy presents as a relatively compact structure with a smooth, centrally concentrated light profile. The morphology appears to be generally elliptical or lenticular, showing a notable lack of prominent spiral arms or distinct dust lanes. The color gradient suggests a population of older stars, contributing to the yellowish hue of the central bulge. There's a hint of bluer light towards the outer regions of the galaxy, potentially indicating ongoing, albeit subdued, star formation activity. The overall shape exhibits a moderate degree of elongation, leaning towards a cigar-like form. No signs of tidal tails or significant morphological distortions are apparent, suggesting the absence of recent major merger events, though there is an indication of minor disturbances in the system's structure.
