The galaxy appears as a moderately luminous object with a distinct, elongated morphology, suggesting an elliptical or lenticular classification. It exhibits a smooth, centrally concentrated light distribution with a gradual decline in brightness towards the outer regions. The color profile suggests a higher proportion of older stellar populations, which is consistent with the galaxy's apparent lack of prominent spiral arm structures. There are no clear indications of ongoing major mergers or tidal disturbances, though minor irregularities cannot be entirely ruled out at this resolution. The object's overall shape is somewhat cigar-shaped with an intermediate roundness. The galaxy exhibits a notable red color, suggesting significant dust content and/or a high fraction of evolved stars.
