This galaxy appears to be an elliptical type, showing a generally smooth, featureless profile. The light distribution is centrally concentrated, with a relatively rapid falloff in brightness away from the core. The galaxy exhibits an elongated morphology, appearing more cigar-shaped than perfectly circular. There is no readily apparent evidence of spiral arm structure or a prominent disk component. The galaxy shows a reddish hue, indicative of an older stellar population and potentially low star formation rate. There are no obvious signs of ongoing mergers or major disturbances affecting the galaxy's structure. Minor irregularities may be present, but it is hard to say for sure at this resolution.
