The galaxy presents as a relatively compact structure, exhibiting an elongated, somewhat irregular morphology. The primary body of the galaxy appears smooth, suggesting an elliptical or lenticular nature, although subtle hints of a disk-like structure are discernible. A faint, bluish region on the upper edge suggests the presence of younger stars and ongoing star formation activity within that localized area. The overall color profile indicates a mix of stellar populations, with the central region tending towards redder hues and potentially containing older stars. Faint tidal features are visible emanating from the main galaxy, possibly indicative of past or ongoing minor mergers or tidal interactions. The galaxy's shape is not perfectly circular; it appears more cigar-shaped, with no clear spiral arm structure apparent. It is likely that any spiral structure has been disrupted by some other event in the past, either a merger or accretion event.
